2. Plan of the Talk What is AGES The AGES volume High density environments –Groups and clusters Low density environments –Galaxy pairs, isolated galaxies and voids Future AGES

3. What is AGES Arecibo Galaxy Environment Survey 200 square degrees in thirteen fields –Four 5 sq. deg. regions –Nine 20 sq. deg. regions Covers environments from the Local Void to the Virgo Cluster 0.7 mJy beam -1 noise level

4. Survey Design Uses the ALFA 7-beam feed array Makes 3 Nyquist-sampled maps with each beam –Provides robustness against beam failure WAPP correlators – 100 MHz bandwidth, 5 km s -1 velocity resolution Mock spectrometers – 300 MHz bandwidth, 4 km s -1 velocity resolution

5. The AGES Volume AGES WAPP cubes are bandpass limited at ~18,000 km s -1 (z ~ 0.06) AGES Mock cubes are bandpass limited at ~45,000 km s -1 (z ~ 0.15) There is a large volume not included in the targeted environment that can be used for ‘blind survey’ science

6. Galaxy at z ~ 0.1

7. Found in 200s of Mock data M HI = 3.6 × 10 10 M ☉, ΔV 50 = 430 km s -1 Such galaxies should be visible to beyond z ~ 0.13 in full-depth data –Most M HI ~ 10 10.5 M ☉ galaxies will be beyond z = 0.1 95 sq. deg. of AGES to be covered with Mock spectrometers

8. AGES HIMF

9. Full sample: α = -1.52±0.05, ϕ = 8.6±1.1 × 10 -3 Mpc -3, M* = 5.1±0.3 × 10 9 M ☉ Field only: α = -1.47±0.06, ϕ = 6.2±0.9 × 10 -3 Mpc -3, M* = 5.6±0.4 × 10 9 M ☉ ~ 2σ steeper than ALFALFA (Martin et al. 2010) or HIPASS (Zwaan et al. 2005) Errors just Poisson noise – including cosmic variance removes inconsistency

10. AGES – High Density Regions Virgo Cluster – 25 sq. deg. completed –See talk by Rhys Taylor Abell 1367 – 5/20 sq. deg. completed N7448 Group – 20 sq. deg. completed N3193 Group – 20 sq. deg. completed –Data currently being reduced Leo Group – 20 sq. deg. in progress

11. Abell 1367

12. Inner strip covering cluster core and infall regions to east and west surveyed (Cortese et al. 2008) Data also used by Scott et al. (2010) and Scott et al. (2012) Infall regions to north and south currently being observed, expected to be completed in 2013

13. NGC 7448

14. Southern 60% published (Davies et al. 2011) Full cube now completed and cataloged (Herbst et al. 2012) Found 10 new dwarfs in the redshift range of the group and 1 in the foreground.

15. AGES – Low Density Regions NGC 7332/9 – 5 sq. deg. completed NGC 4302/4298 – 20 sq. deg. not started NGC 1156 – 5 sq. deg. completed UGC 2082 – 5 sq. deg. completed NGC 5523 – 20 sq. deg. in progress Local Void – 20 sq. deg. not started

16. NGC 7332/9 Published in Minchin et al. (2010) NGC 7339: a spiral with known HI NGC 7332: a lenticular with ionized gas Found two M HI ~ 10 7 M ☉ dwarfs nearby

17. NGC 7332/9

18. Published in Minchin et al. (2010) NGC 7339: a spiral with known HI NGC 7332: a lenticular with ionized gas Found two M HI ~ 10 7 M ☉ dwarfs nearby Found solid evidence that NGC 7332 is accreting gas from NGC 7339

19. NGC 7332/9

20. NGC 1156 & UGC 2082 Minchin et al. (2010); Taber et al. (2011) Closest M HI > 10 9 M ☉ isolated galaxies Selection criteria make companions with M HI > 10 7.8 M ☉ unlikely AGES has 1 – 1.6 decades of sensitivity below this to look for dwarfs Found one M HI ~ 10 6 M ☉ companion to each galaxy – fewer than expected

21. NGC 1156 & UGC 2082

23. 3σ underdensity

24. NGC 1156 & UGC 2082 7σ underdensity

25. NGC 1156 & UGC 2082 5σ underdensity

26. Future AGES Wider survey of the Virgo Cluster to AGES depth Deep survey of Virgo and other environments to see what is missed Targeted survey for low-mass dwarfs around isolated galaxies